Cosmic Microwave Background non-Gaussian signatures from analytical texture models

Details Cosmic Microwave Background non-Gaussian signatures from analytical texture models Cosmic Microwave Background non-Gaussian signatures from analytical texture models

1996-01-12

arxiv.org/abs/astro-ph/9601069v2

Phys.Rev. D54 (1996) 4750-4756

Astronomy and Astrophysics

Astrophysics

13 pp, RevTeX, 4 PostScript figures, to appear in Phys.Rev.D

Scientific paper

10.1103/PhysRevD.54.4750

Using an analytical model for the Cosmic Microwave Background anisotropies produced by textures, we compute the resulting collapsed three--point correlation function and the {\it rms} expected value due to the cosmic variance. We apply our calculations to the {\sl COBE}--DMR experiment and test the consistency of the model with the observational results. We also show that an experiment with smaller angular resolution can put bounds to the model parameters.

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